FSR 1167

(MWSC 980)

0.14 UTI

0.0

C_N

0.06

C_dens

0.12

C_C3

0.25

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 19

Radius (P>50% members) 8.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.06 Very loose
C_C3 0.12 Very low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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FSR 1167 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.50 kpc) differs significantly from the median photometric distance (~2.33 kpc).

Note: This object shares a significant percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Moderate extinction Old

Data

🔍 Search references for FSR 1167 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	101.572	-10.978	0.286	-0.942	0.889	–
Just et al.	2023	101.581	-10.983	–	–	–	–
Kharchenko et al.	2016	101.581	-10.983	–	–	–	–
Kharchenko et al.	2013	101.587	-10.985	–	1.55	-0.36	–
Froebrich et al.	2007	101.617	-10.984	–	–	–	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
Just et al.	2023	–	–	–	2427	–	307	–	–
Kharchenko et al.	2016	2.33	1.62	–	2427	–	–	–	–
Kharchenko et al.	2013	2.33	1.62	–	2427	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 1166	56.0	101.54	-10.98	0.26	-0.96	0.92	73.34	0.03

💡 Note: The % column shows the percentage of members that FSR 1167 shares with each listed object.

Visualization

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